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Kiss, C.; Müller, T. G.; Marton, G.; Szakáts, R.; Pál, A.; Molnár, L.; Vilenius, E.; Rengel, M.; Ortiz, J. L.; Fernández-Valenzuela, E.: The visible and thermal light curve of the large Kuiper belt object (50000) Quaoar★. Astronomy and Astrophysics 684, p. A50 (2024)
Rengel, M.: Editorial: Editor's challenge in planetary science: the future of planetary exploration and the next generation of planetary missions. Frontiers in Astronomy and Space Sciences 11, p. 1370464 (2024)
Rengel, M.; Adamczewski, J.: Radiative transfer and inversion codes for characterizing planetary atmospheres: an overview. Frontiers in Astronomy and Space Sciences 10, p. 1176740 (2023)
Rengel, M.; Adamczewski, J.: Radiative transfer and inversion codes for characterizing planetary atmospheres: an overview. Frontiers in Astronomy and Space Sciences 10, p. 1176740 (2023)
Howell, S. B.; Izmodenov, V.; Kopeikin, S. M.; Marziani, P.; Puzzarini, C.; Rengel, M.; McIntosh, S. W.; Fraix-Burnet, D.; Kanik, I.: Editorial: Frontiers in astronomy and space sciences: Rising stars. Frontiers in Astronomy and Space Sciences 9, p. 991696 (2022)
Rengel, M.; Shulyak, D.; Hartogh, P.; Sagawa, H.; Moreno, R.; Jarchow, C.: Ground-based HCN submillimetre measurements in Titan's atmosphere: an intercomparison with Herschel observations. Astronomy and Astrophysics 658, p. A88 (2022)
Fossati, L.; Shulyak, D.; Sreejith, A. G.; Koskinen, T.; Young, M. E.; Cubillos, P. E.; Lara, L. M.; France, K.; Rengel, M.; Cauley, P. W.et al.; Turner, J. D.; Wyttenbach, A.; Yan, F.: A data-driven approach to constraining the atmospheric temperature structure of the ultra-hot Jupiter KELT-9b. Astronomy and Astrophysics 643, A131 (2020)
Piccialli, A.; Rathbun, J. A.; Levasseur-Regourd, A.-C.; Määttänen, A.; Milillo, A.; Rengel, M.; Rotundi, A.; Taylor, M.; Witasse, O.; Altieri, F.et al.; Drossart, P.; Vandaele, A. C.: Participation of women scientists in ESA solar system missions: a historical trend. Advances in Geosciences 53, pp. 169 - 182 (2020)
Shulyak, D.; Lara, L. M.; Rengel, M.; Nemec, N.-E.: Stellar impact on disequilibrium chemistry and observed spectra of hot Jupiter atmospheres. Astronomy and Astrophysics 639, A48 (2020)
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, ...