Anand, A.; Spitzer, F.; Hopp, T.; Windmill, R.; Kruttasch, P.; Burkhardt, C.; Dauphas, N.; Greenwood, R.; Hofmann, B.; Mezger, K.et al.; Kleine, T.: Isotopic evidence for a common parent body of IIG and IIAB iron meteorites. Geochimica et Cosmochimica Acta 382, pp. 118 - 127 (2024)
Hellmann, J. L.; Van Orman, J. A.; Kleine, T.: Hf-W isotope systematics of enstatite chondrites: Parent body chronology and origin of Hf-W fractionations among chondritic meteorites. Earth and Planetary Science Letters 626, p. 118518 (2024)
Jansen, C. A.; Burkhardt, C.; Marrocchi, Y.; Schneider, J. M.; Wölfer, E.; Kleine, T.: Condensate evolution in the solar nebula inferred from combined Cr, Ti, and O isotope analyses of amoeboid olivine aggregates. Earth and Planetary Science Letters 627, p. 118567 (2024)
Mazza, S. E.; Gaschnig, R. M.; Rudnick, R. L.; Kleine, T.: Tungsten stable isotope composition of the upper continental crust. Geochimica et Cosmochimica Acta 370, pp. 161 - 172 (2024)
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 and Planetary Science 59, pp. 778 - 788 (2024)
Archer, G. J.; Budde, G.; Worsham, E. A.; Stracke, A.; Jackson, M. G.; Kleine, T.: Origin of 182W Anomalies in Ocean Island Basalts. Geochemistry, Geophysics, Geosystems 24, p. e2022GC010688 (2023)
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)
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 Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.