Basilevsky, A. T.; Mall, U.; Keller, H. U.; Skorov, Y. V.; Hviid, S. F.; Mottola, S.; Krasilnikov, S. S.; Dabrowski, B.: Geologic analysis of the Rosetta NavCam, Osiris and ROLIS images of the comet 67P/Churyumov-Gerasimenko nucleus. Planetary and Space Science 137, pp. 1 - 19 (2017)
Marschall, R.; Mottola, S.; Su, C. C.; Liao, Y.; Rubin, M.; Wu, J. S.; Thomas, N.; Altwegg, K.; Sierks, H.; Ip, W.-H.et al.; Keller, H. U.; Knollenberg, J.; Kuehrt, E.; Lai, I. L.; Skorov, Y.; Jorda, L.; Preusker, F.; Scholten, F.; Vincent, J.-B.; The OSIRIS Team: Cliffs versus plains: Can ROSINA/COPS and OSIRIS data of comet 67P/Churyumov-Gerasimenko in autumn 2014 constrain inhomogeneous outgassing? Astronomy and Astrophysics 605, A112 (2017)
Skorov, Y. V.; Rezac, L.; Hartogh, P.; Keller, H. U.: Is near-surface ice the driver of dust activity on 67P/Churyumov-Gerasimenko? Astronomy and Astrophysics 600, A142 (2017)
Basilevsky, A. T.; Krasilnikov, S. S.; Shiryaev, A. A.; Mall, U.; Keller, H. U.; Skorov, Y. V.; Mottola, S.; Hviid, S. F.: Estimating the Strength of the Nucleus Material of Comet 67P Churyumov-Gerasimenko. Solar System Research 50, pp. 225 - 234 (2016)
Liao, Y.; Su, C. C.; Marschall, R.; Wu, J. S.; Rubin, M.; Lai, I. L.; Ip, W. H.; Keller, H. U.; Knollenberg, J.; Kuehrt, E.et al.; Skorov, Y. V.; Thomas, N.: 3D Direct Simulation Monte Carlo Modelling of the Inner Gas Coma of Comet 67P/Churyumov-Gerasimenko: A Parameter Study. Earth, Moon and Planets 117 (1), pp. 41 - 64 (2016)
Gundlach, B.; Blum, J.; Keller, H. U.; Skorov, Y. V.: What drives the dust activity of comet 67P/Churyumov-Gerasimenko? Astronomy and Astrophysics 583, A12 (2015)
Keller, H. U.; Mottola, S.; Skorov, Y.; Jorda, L.: The changing rotation period of comet 67P/Churyumov-Gerasimenko controlled by its activity. Astronomy and Astrophysics 579, L5 (2015)
Ivanova, O. V.; Skorov, Y. V.; Korsun, P. P.; Afanasiev, V. L.; Blum, J.: Observations of the long-lasting activity of the distant Comets 29P Schwassmann-Wachmann 1, C/2003 WT42 (LINEAR) and C/2002 VQ94 (LINEAR). Icarus 211 (1), pp. 559 - 567 (2011)
Skorov, Y. V.; van Lieshout, R.; Blum, J.; Keller, H. U.: Activity of comets: Gas transport in the near-surface porous layers of a cometary nucleus. Icarus 212 (2), pp. 867 - 876 (2011)
Skorov, Y. V.; Keller, H. U.; Rodin, A. V.: Optical properties of aerosols in Titan's atmosphere: Large fluffy aggregates. Planetary and Space Science 58 (14-15), pp. 1802 - 1810 (2010)
Skorov, Y. V.; Keller, H. U.; Rodin, A. V.: Optical properties of aerosols in Titan's atmosphere. Planetary and Space Science 56 (5), pp. 660 - 668 (2008)
Skorov, Y. V.; Markelov, G. N.; Keller, H. U.: Direct statistical simulation of the near-surface layers of the cometary atmosphere. I. A spherical nucleus. Solar System Research 38 (6), pp. 455 - 475 (2004)
Davidsson, B. J. R.; Skorov, Y. V.: On the light-absorbing surface layer of cometary nuclei - II. Thermal modeling. Icarus 159 (1), pp. 239 - 258 (2002)
Skorov, Y. V.; Keller, H. U.; Jorda, L.; Davidsson, B. J. R.: Thermophysical modelling of Comet P/Borrelly: Effects of volume energy absorption and volume sublimation. Earth, Moon and Planets 90, pp. 293 - 303 (2002)
Skorov, Y. V.; Kömle, N. I.; Keller, H. U.; Kargl, G.; Markiewicz, W. J.: A model of heat and mass transfer in a porous cometary nucleus based on a kinetic treatment of mass flow. Icarus 153 (1), pp. 180 - 196 (2001)
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".
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.