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Medvedev, A. S.; Yiğit, E.; Hartogh, P.: Ion friction and quantification of the geomagnetic influence on gravity wave propagation and dissipation in the thermosphere-ionosphere. Journal of Geophysical Research: Space Physics 122 (12), pp. 464 - 475 (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)
Hartogh, P.; Ilyushin, Y. A.: A passive low frequency instrument for radio wave sounding the subsurface oceans of the Jovian icy moons: An instrument concept. Planetary and Space Science 130, pp. 30 - 39 (2016)
Kuroda, T.; Medvedev, A. S.; Yiğit, E.; Hartogh, P.: Global distribution of gravity wave sources and fields in the Martian atmosphere during equinox and solstice inferred from a high-resolution general circulation model. Journal of the Atmospheric Sciences 73, pp. 4895 - 4909 (2016)
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Villanueva, G. L.; Altieri, F.; Clancy, R. T.; Encrenaz, T.; Fouchet, T.; Hartogh, P.; Lellouch, E.; Lopéz-Valverde, M. A.; Mumma, M. J.; Novak, R. E.et al.; Smith, M. D.; Vandaele, A.-C.; Wolff, M. J.; Ferruit, P.; Milam, S. N.: Unique Spectroscopy and Imaging of Mars with the James Webb Space Telescope. Publications of the Astronomical Society of Pacific 128 (959), 018004 (2016)
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Cavalié, T.; Dobrijevic, M.; Fletcher, L. N.; Loison, L.-C.; Hickson, K. M.; Hue, V.; Hartogh, P.: Photochemical response to the variation of temperature in the 2011-2012 stratospheric vortex of Saturn. Astronomy and Astrophysics 580, A55 (2015)
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Encrenaz, T.; Tinetti, G.; Tessenyi, M.; Drossart, P.; Hartogh, P.; Coustenis, A.: Transit spectroscopy of exoplanets from space: how to optimize the wavelength coverage and spectral resolving power. Experimental Astronomy 40, pp. 523 - 543 (2015)
Kuroda, T.; Medvedev, A. S.; Yiğit, E.; Hartogh, P.: A global view of gravity waves in the Martian atmosphere inferred from a high-resolution general circulation model. Geophysical Research Letters 42, pp. 9213 - 9222 (2015)
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".