Yiğit, E.; Medvedev, A. S.; Hartogh, P.: Variations of the Martian Thermospheric Gravity-wave Activity during the Recent Solar Minimum as Observed by MAVEN. The Astrophysical Journal 920 (2), 69 (2021)
Benmahi, B.; Cavalié, T.; Dobrijevic, M.; Biver, N.; Bermudez-Diaz, K.; Sandqvist, A.; Lellouch, E.; Moreno, R.; Fouchet, T.; Hue, V.et al.; Hartogh, P.; Billebaud, F.; Lecacheux, A.; Hjalmarson, Å.; Frisk, U.; Olberg, M.: Monitoring of the evolution of H2O vapor in the stratosphere of Jupiter over an 18-yr period with the Odin space telescope. Astronomy and Astrophysics 641, A140 (2020)
Ilyushin, Y. A.; Hartogh, P.: Submillimeter Wave Instrument radiometry of the Jovian icy moons: Numerical simulation of the microwave thermal radiative transfer and Bayesian retrieval of the physical properties. Astronomy and Astrophysics 644, A24 (2020)
Skorov, Y. V.; Keller, H. U.; Mottola, S.; Hartogh, P.: Near-perihelion activity of comet 67P/Churyumov–Gerasimenko. A first attempt of non-static analysis. Monthly Notices of the Royal Astronomical Society 494 (3), pp. 3310 - 3316 (2020)
Wirström, E. S.; Bjerkeli, P.; Rezac, L.; Brinch, C.; Hartogh, P.: Effect of the 3D distribution on water observations made with the SWI - I. Ganymede. Astronomy and Astrophysics 637, A90 (2020)
Zhao, Y.; Rezac, L.; Hartogh, P.; Ji, J.; Marschall, R.; Keller, H. U.: Constraining spatial pattern of early activity of comet 67P/C–G with 3D modelling of the MIRO observations. Monthly Notices of the Royal Astronomical Society 494 (2), pp. 2374 - 2384 (2020)
Biver, N.; Bockelée-Morvan, D.; Hofstadter, M.; Lellouch, E.; Choukroun, M.; Gulkis, S.; Crovisier, J.; Schloerb, F. P.; Rezac, L.; von Allmen, P.et al.; Lee, S.; Leyrat, C.; Ip, W. H.; Hartogh, P.; Encrenaz, P.; Beaudin, G.; the MIRO Team: Long-term monitoring of the outgassing and composition of comet 67P/Churyumov-Gerasimenko with the Rosetta/MIRO instrument. Astronomy and Astrophysics 630, A19 (2019)
Jesch, D.; Medvedev, A. S.; Castellini, F.; Yiğit, E.; Hartogh, P.: Density Fluctuations in the Lower Thermosphere of Mars Retrieved From the ExoMars Trace Gas Orbiter (TGO) Aerobraking. Atmosphere 10 (10), 620 (2019)
Marshall, D. W.; Rezac, L.; Hartogh, P.; Zhao, Y.; Attree, N.: Interpretation of heliocentric water production rates of comets. Astronomy and Astrophysics 623, A120 (2019)
Rezac, L.; Zhao, Y.; Hartogh, P.; Ji, J.; Marshall, D. W.; Shi, X.: Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko. Astronomy and Astrophysics 630, A34 (2019)
Shaposhnikov, D. S.; Medvedev, A. S.; Rodin, A. V.; Hartogh, P.: Seasonal Water “Pump” in the Atmosphere of Mars: Vertical Transport to the Thermosphere. Geophysical Research Letters 46 (8), pp. 4161 - 4169 (2019)
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.
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".