Guettler, C.; Rose, M.; Sierks, H.; Macher, W.; Zivithal, S.; Blum, J.; Laddha, S.; Gundlach, B.; Kargl, G.: Simulation and experiment of gas diffusion in a granular bed. Monthly Notices of the Royal Astronomical Society 524, pp. 6114 - 6123 (2023)
Laddha, S.; Macher, W.; Kargl, G.; Zivithal, S.; Blum, J.; Gundlach, B.; Güttler, C.; Sierks, H.; Rose, M.: Validation of gas flow experiments for porous media by means of computer simulations. Measurement Science and Technology 34, p. 045012 (2023)
Davidsson, B. J. R.; Schloerb, F. P.; Fornasier, S.; Oklay, N.; Gutiérrez, P. J.; Buratti, B. J.; Chmielewski, A. B.; Gulkis, S.; Hofstadter, M. D.; Keller, H. U.et al.; Sierks, H.; Güttler, C.; Küppers, M.; Rickman, H.; Choukroun, M.; Lee, S.; Lellouch, E.; Lethuillier, A.; Da Deppo, V.; Groussin, O.; Kührt, E.; Thomas, N.; Tubiana, C.; El-Maarry, M. R.; La Forgia, F.; Mottola, S.; Pajola, M.: CO2-driven surface changes in the Hapi region on Comet 67P/Churyumov-Gerasimenko. Monthly Notices of the Royal Astronomical Society 516, pp. 6009 - 6040 (2022)
Cambianica, P.; Cremonese, G.; Fulle, M.; Simioni, E.; Naletto, G.; Pajola, M.; Lucchetti, A.; Penasa, L.; Massironi, M.; Frattin, E.et al.; Güttler, C.; Sierks, H.; Tubiana, C.: Long-term measurements of the erosion and accretion of dust deposits on comet 67P/Churyumov-Gerasimenko with the OSIRIS instrument. Monthly Notices of the Royal Astronomical Society 504 (2), pp. 2895 - 2910 (2021)
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Franceschi, M.; Penasa, L.; Massironi, M.; Naletto, G.; Ferrari, S.; Fondriest, M.; Bodewits, D.; Güttler, C.; Lucchetti, A.; Mottola, S.et al.; Pajola, M.; Toth, I.; Deller, J.; Sierks, H.; Tubiana, C.: Global-scale brittle plastic rheology at the cometesimals merging of comet 67P/Churyumov–Gerasimenko. Proceedings of the National Academy of Sciences of the United States of America 117 (19), pp. 10181 - 10187 (2020)
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Van Hoang, H.; Fornasier, S.; Quirico, E.; Hasselmann, P. H.; Barucci, M. A.; Sierks, H.; Tubiana, C.; Guettler, C.: Spectrophotometric characterization of the Philae landing site and surroundings with the Rosetta/OSIRIS cameras. Monthly Notices of the Royal Astronomical Society 498 (1), pp. 1221 - 1238 (2020)
Feller, C.; Fornasier, S.; Ferrari, S.; Hasselmann, P. H.; Barucci, A.; Massironi, M.; Deshapriya, J. D. P.; Sierks, H.; Naletto, G.; Lamy, P. L.et al.; Rodrigo, R.; Koschny, D.; Davidsson, B. J. R.; Bertaux, J.-L.; Bertini, I.; Bodewits, D.; Cremonese, G.; Da Deppo, V.; Debei, S.; De Cecco, M.; Fulle, M.; Gutiérrez, P. J.; Güttler, C.; Ip, W.-H.; Keller, H. U.; Lara, L. M.; Lazzarin, M.; López-Moreno, J. J.; Marzari, F.; Shi, X.; Tubiana, C.; Gaskell, B.; La Forgia, F.; Lucchetti, A.; Mottola, S.; Pajola, M.; Preusker, F.; Scholten, F.: Rosetta/OSIRIS observations of the 67P nucleus during the April 2016 flyby: high-resolution spectrophotometry. Astronomy and Astrophysics 630, A19 (2019)
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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, ...