Drazkowska, J.; Dullemond, C. P.: Planetesimal formation during protoplanetary disk buildup (Corrigendum). Astronomy and Astrophysics 671, p. C10 (2023)
Stammler, S. M.; Lichtenberg, T.; Drazkowska, J.; Birnstiel, T.: Leaky dust traps: How fragmentation impacts dust filtering by planets. Astronomy & Astrophysics 670, p. L5 (2023)
Lau, T. C. H.; Drazkowska, J.; Stammler, S. M.; Birnstiel, T.; Dullemond, C. P.: Rapid formation of massive planetary cores in a pressure bump. Astronomy and Astrophysics 668, p. A170 (2022)
Choukroun, M.; Altwegg, K.; Kührt, E.; Biver, N.; Bockelée-Morvan, D.; Drazkowska, J.; Hérique, A.; Hilchenbach, M.; Marschall, R.; Pätzold, M.et al.; Taylor, M. G. G. T.; Thomas, N.: Dust-to-Gas and Refractory-to-Ice Mass Ratios of Comet 67P/Churyumov-Gerasimenko from Rosetta Observations. Space Science Reviews 216, 44 (2020)
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.